Statistics – Computation
Scientific paper
Oct 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...205..347k&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 205, no. 1-2, Oct. 1988, p. 347-353.
Statistics
Computation
25
Electron Density Profiles, Ground State, Neutron Stars, Nuclear Binding Energy, Pulsars, Stellar Magnetic Fields, Computational Astrophysics, Coulomb Collisions, Density Distribution, Iron, Magnetic Flux
Scientific paper
The ground state binding energy, the ionisation energy, the electron density distribution and the quadrupole moment of iron atoms in strong magnetic fields (1 - 8×1012G) have been calculated using the density functional method. The authors have also performed calculations of the ground state energy for helium, carbon, and oxygen atoms, and for the helium-like ions of carbon (C4+), oxygen (O6+) and iron (Fe24+), respectively. Finally, they have calculated the binding energy (per atom) of a hexagonal iron crystal due to the quadrupole-quadrupole interaction of the deformed iron atoms.
Hillebrandt Wolfgang
Koessl D.
Mueller Ewald
Wolff R. G.
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